@article{oai:nagoya.repo.nii.ac.jp:00019699,
 author = {柿沼, 隆清 and 高柳, 利男 and 太陽電波研究室一同 and Kakinuma, Takakiyo and Takayanagi, Toshio and other members of Radio Astronomy Section},
 issue = {1-2},
 journal = {空電研究所報告},
 month = {May},
 note = {The results of observations by 3750 and 9400 Mc/s radiometers are tabulated. The daily flux density at both frequencies has a correlation coefficient of 0.95, and the S-component at 9400 Mc/s is 0.8 times as large as that at 3750 Mc/s. The sense of polarization at both frequencies is similar. The percentage polarization referring to the S-component of an isolated radio spot occasionally exceeds 30 percent at 9400 Mc/s, which is much larger than that at 3750 Mc/s. Some bursts show yet a remarkable structure of frequency spectrum at these super-high-frequencies. The observations with an 8-element interferometer have been made for five hours every day for locating sources of outstanding occurrences. A burst occasionally occurs in an emissive region where no intense radiation is usually observed.},
 pages = {66--99},
 title = {太陽電波の観測と二三の考察},
 volume = {7},
 year = {1957}
}